![[Operator logo]](/static/img/logo_medium.png){kind=logo}
Metadata
Identifier
Cite this
Description
Keywords
astronomical-software
![[Logo]](http://voparis-srv-paris.obspm.fr/logos/PADC_small.png)
| Tablename | Tableinfo | Table desc. | Res desc. |
|---|---|---|---|
| amdadb.epn_core | Table Info | Planetary and heliophysics plasma data at CDPP/AMDA | Planetary and heliophysics plasma data at CDPP/AMDA |
| apis.epn_core | Table Info | EpnCore table for APIS service | Planetary aurorae are powerful emissions radiated from auroral regions of magnetized planets by accelerated charged particles, in a wide range of wavelengths (from radio to X-rays). The UV range in particular is adequate to measure collisionaly excited transitions of H and H2, the dominant species in the upper atmosphere of giant planets, produced by precipitating auroral particles, and benefits a good angular resolution. Auroral UV observations therefore provide a rich source of informations on planetary atmospheres and magnetospheres. They also offer a unique diagnostic to remotely probe the solar wind activity throughout the heliosphere. |
| basecom.epn_core | Table Info | N/A | Since 1973, the 18-cm lines of the OH radical have been systematically observed in a number of comets with the Nançay radio telescope. This allowed an evaluation of the cometary water production rates and their evolution with time, as well as a study of several physical processes: the excitation mechanisms of the OH radio lines, the expansion of the cometary atmospheres, their anisotropy in relation with non-gravitational forces, the Zeeman effect in relation with the cometary magnetic field. The Nançay observations of 53 cometary apparitions between 1982 and 2009 are now organized in this database. |
| bass2000.epn_core | Table Info | EPNcore table of BASS2000, a Solar survey archive: Images, movies of full Sun from groundbased instruments: Spectroheliographs of Meudon and Coimbra, RadioHeliograph and Decametric Array of Nancay, CLIMSO, USET | BASS2000 archives and distributes groundbased solar observations provided by various instruments: the RadioHeliograph and Decametric Array of Nancay, Spectroheliographes of Meudon and Coimbra, CLIMSO, the Coronographe of Pic du Midi, the Uccle Solar Equatorial Table (USET). It is also WDC-Solar Activity, Regular Member of ICSU World Data system. |
| bdip.epn_core | Table Info | Planetary Images Database | One Century of Planetary Images ------------------------------- The database of planetary images (BDIP) comes from the digitization of photographs collected and preserved by the Center for Photographic Documentation of the planets held by the IAU at the Meudon Observatory in 1961 under the the curation of J.H. Focas (IAUC, 12th General Assembly, Report 1964). A similar center was established at the Lowell Observatory in Arizona, under the responsibility of W.A. Baum. The photographs were duplicated between the two centers. Approximately 8400 photographs of Mars, Venus, Mercury, Jupiter and Saturn, acquired between 1890 and 1977, are kept at LESIA. They remain available for research on justified request. The digitization of these planetary photographs was performed by scanning between 1998 and 2000 by the staff of the Documentation Center (R. Boyer, E. Neyvoz et al), in the framework of a project proposed to the Scientific Council of the Paris Observatory by P. Drossart. Care was taken to preserve the best possible definition and photometric linearity of photographs during the scanning procedure. Storage was done using different image formats (JPEG, GIF and TIFF ie, lossy, lossless and uncompressed). Improved techniques for mass storage and network distribution today allow us to provide access to the highest definition images, thereby facilitating research on the evolution of planets, at asecular time scale. Scientific interest ------------------- The scientific interest of the photographic database mainly concerns planetary atmospheric evolution of Mars, Jupiter, Saturn and Venus. The evolution of the Martian storms, or the polar caps on Mars, the survey of storms observed on Saturn, or features like the Great Red Spot of Jupiter or oval white spots are among the subjects which triggered on photographs. Such studies can be refined today thanks to digital pictures (Sanchez-Lavega and Battaner, A and A Suppl. Ser., 64, 287, 1986). Some images of Mercury are also available. |
| bdip.observatories | Table Info | Observatory names | One Century of Planetary Images ------------------------------- The database of planetary images (BDIP) comes from the digitization of photographs collected and preserved by the Center for Photographic Documentation of the planets held by the IAU at the Meudon Observatory in 1961 under the the curation of J.H. Focas (IAUC, 12th General Assembly, Report 1964). A similar center was established at the Lowell Observatory in Arizona, under the responsibility of W.A. Baum. The photographs were duplicated between the two centers. Approximately 8400 photographs of Mars, Venus, Mercury, Jupiter and Saturn, acquired between 1890 and 1977, are kept at LESIA. They remain available for research on justified request. The digitization of these planetary photographs was performed by scanning between 1998 and 2000 by the staff of the Documentation Center (R. Boyer, E. Neyvoz et al), in the framework of a project proposed to the Scientific Council of the Paris Observatory by P. Drossart. Care was taken to preserve the best possible definition and photometric linearity of photographs during the scanning procedure. Storage was done using different image formats (JPEG, GIF and TIFF ie, lossy, lossless and uncompressed). Improved techniques for mass storage and network distribution today allow us to provide access to the highest definition images, thereby facilitating research on the evolution of planets, at asecular time scale. Scientific interest ------------------- The scientific interest of the photographic database mainly concerns planetary atmospheric evolution of Mars, Jupiter, Saturn and Venus. The evolution of the Martian storms, or the polar caps on Mars, the survey of storms observed on Saturn, or features like the Great Red Spot of Jupiter or oval white spots are among the subjects which triggered on photographs. Such studies can be refined today thanks to digital pictures (Sanchez-Lavega and Battaner, A and A Suppl. Ser., 64, 287, 1986). Some images of Mercury are also available. |
| cassini_rpws.epn_core | Table Info | VESPA/EPNcore table for the Cassini/RPWS Kronos Database | Cassini/RPWS Kronos Database |
| csa.epn_core | Table Info | N/A | The British Astronomical Association has been collecting observations since 1890. Here we provide access to Comet Observations, both visual and CCD. Informations for alternate target name come from caero resolver, and ephemeris from miriad, both services are from the coutesy og IMCCE-Observatoire de Paris-PSL |
| cubesat_project.epn_core | Table Info | N/A | "Example telemetry data retrived from github of an open source Cubesat project https://github.com/stanford-ssi/sapling-data/blob/main/sapling-giganteum/decoded_telem.csv" |
| esor.main | Table Info | N/A | all the image have been resampled and reprojected TAN |
| exoplanet.epn_core | Table Info | Encyclopedia of extrasolar planet | Encyclopedia of extrasolar planet |
| expres.epn_core | Table Info | N/A | ExPRES Simulation service catalog |
| gmap.epn_core | Table Info | N/A | GMap provides planetary geological maps of different Solar System bodies, developed by an open community, reviewed by scientists. GMap inherits its data model from Planmap, most of the maps provide morphological information, some provide stratigraphic or compositional information too. Each original data packages provided is a collection of vector, raster, and, in some cases, 3D models. In this EPN-TAP service, the data records (`granule_uid`) refer to each of the data files in the whole of GMAP archive, grouped by (`granule_gid`) the data package --map-- they compose. |
| hess_dr.obscore | Table Info | IVOA ObsCore description of event lists for observations in the H.E.S.S. DL3 public test data release 1 | The release consists of event lists and instrument response functions for observations of various well-known gamma-ray sources (the Crab nebula, PKS 2155-304, MSH 15-52, RX J1713.7-3946) as well as observations of empty fields for background modeling. |
| hfc1ar_backup.epn_core | Table Info | Active regions of the Sun from Heliophysics Feature Catalogue (HFC). | Description of active regions automatically detected from SOHO/MDI images using SMART code, and from SOHO/EIT and SDO/AIA images, using SPOCA-AR code. Detections are available from 1996 till now. In addition to active region description a chain code gives its contour. |
| hfc1ar.epn_core | Table Info | Active regions of the Sun from Heliophysics Feature Catalogue (HFC). | Description of active regions automatically detected from SOHO/MDI images using SMART code, and from SOHO/EIT and SDO/AIA images, using SPOCA-AR code. Detections are available from 1996 till now. In addition to active region description a chain code gives its contour. |
| hfc1sunspots.epn_core | Table Info | N/A | |
| hfc1t3.epn_core | Table Info | type 3 events of the sun from helio database. | Solar type 3 events extracted from Heliophysics Feature Catalog. |
| hst_asteroids.epn_core | Table Info | N/A | HST spectra of asteroids extracted from the CADC database catalogue (with daily updates). Data are linked to the CADC repository, with file names common to all HST archives. Both calibrated and derived products are included. The main target is identified. Physical ephemeris and thumbnails are provided when available. Files and previews are not accessible during the proprietary period. |
| hst_planeto.epn_core | Table Info | N/A | HST observations of planets, dwarf planets, and satellites, extracted from the CADC database catalogue (with daily updates). Data are linked to the CADC repository, with file names common to all HST archives. Both calibrated and derived products are included. The main target is identified. Physical ephemeris and thumbnails are provided when available. Files and previews are not accessible during the proprietary period. |
| iitatehf.epn_core | Table Info | Iitate log periodic Radio antenna High Resolution data | TBD |
| iks.epn_core | Table Info | N/A | Measurements of comet Halley in the spectral channel of IKS on board the Vega-1 spacecraft. Data are retrieved from the PDS Small Bodies Node data set (2011 reformatted version) and updated. The data set consists in 101 tables providing the radiance spectrum of comet Halley from various distances, plus two composite spectra. For details and further references, see: Combes M. et al., 1988, The 2.5-12 micron Spectrum of Comet Halley from the IKS-VEGA Experiment, Icarus, 76, 404-436 [1988Icar...76..404C] |
| i_lofar.epn_core | Table Info | N/A | Low Frequency radio observation from the Irish LOFAR (I-LOFAR, or IE613) station, using the KAIRA (Kilpisjarvi Atmospheric Imaging Receiver Array). This service provides access to Solar observations. |
| impex.epn_core | Table Info | IMPEx Simulation Data | IMPEx simulation runs provided by FMI, LATMOS and SINP |
| ipda.IPDA | Table Info | N/A | This service lists some data access system for Solar System data. Currently an assessment study at IPDA |
| Tablename | Tableinfo | Table desc. | Res desc. |
| ivoa.ObsCore | Table Info | The IVOA-defined obscore table, containing generic metadata for datasets within this datacenter. | Definition and support code for the ObsCore data model and table. |
| juno_waves.epn_core | Table Info | N/A | Juno/Waves database at LESIA. This collection contains L3 data products. This collection is maintained by the MASER team. |
| jwst.epn_core | Table Info | N/A | DESCRIPTION |
| lathys.epn_core | Table Info | IMPEx Simulation Data | IMPEx simulation runs provided by LATMOS |
| luckystar.epn_core | Table Info | N/A | Draft version from catalogue date found here: http://occultations.ct.utfpr.edu.br/results/ |
| lunar_craters.epn_core | Table Info | Lunar crater catalogue | This is the Moon Crater Database v1 by Salamunićcar et al, 2012, http://doi.org/10.1016/j.pss.2011.09.003 - an EPN-TAP version of their LU60645GT catalogue. The catalogues by McDowell, Rodionova, and Head have been integrated with the results of a Crater Shape-based interpolation crater detection algorithm and Lunar Orbiter Laser Altimeter (LOLA) data. This catalogue is globally complete up to ∼D≥8 km. The original version is distributed by USGS: https://astrogeology.usgs.gov/search/map/Moon/Research/Craters/GoranSalamuniccar_MoonCraters |
| m4ast.epn_core | Table Info | compiled database for asteroid spectra in the visible and NIR regions | compiled database for asteroid spectra in the visible and NIR regions |
| meteor_showers.epn_core | Table Info | N/A | The ephemeris were produced by simulating the ejection of meteoroids from the sunlit hemisphere of cometary nuclei, typically from 0 to 3 au, followed by the propagation of orbits of meteoroids in the Solar System, taking into account the gravitation of the Sun, the 8 planets, Pluto, and the Moon, as well as the radiation pressure and the Poynting-Robertson drag. Note that asteroid parent bodies were considered as active (i.e. comet-like bodies) even if they are not active today. The showers are predicted when a planet enters a large enough set of meteoroids, at a distance less than typically 0.01 au. See Vaubaillon J., Colas F., Jorda L. 2005 A new method to predict meteor showers. I. Description of the model, Astronomy and Astrophysics, Volume 439/2 p.751-760, as well as: Vaubaillon J. 2017 A confidence index for forecasting of meteor showers, Planetary and Space Science, Volume 143 p.78-82 |
| missions_ipda.epn_core | Table Info | N/A | This service lists some datasets for the Solar System (from R. Beebe IPDA project, 2022). Currently an assessment study at IPDA |
| moonsprop.epn_core | Table Info | N/A | This service provides the physical and dynamical characteristics of natural satellites in the Solar System: size, mass, rotational properties, magnitude and albedo, orbital elements. These quantities are taken from various publications listed under the bib_reference parameter. These data will be updated as new values are published. |
| naroo.main | Table Info | N/A | TBD |
| nda.epn_core | Table Info | N/A | Decametric radio observation from Nancay decameter array. The Nancay Decameter Array (NDA) at the Station de Radioastronomie de Nancay (SRN) is a phased array of 144 "Teepee" helicoidal antenna, half of which being Right Handed (RH) polarized and the other half being Left Handed (LH) polarized. Four receivers are currently connected to the NDA, sampling data in spectral ranges within 5 to 80 MHz. |
| nrh.epn_core | Table Info | N/A | Data of Nançay Radioheliograph instrument |
| orfees.epn_core | Table Info | N/A | Données de l'instrument ORFEES (Observations Radiospectrales pour FEDOME et l'Etude des Eruptions Solaires) |
| parsec.epn_core | Table Info | N/A | Observational data collected by Europlanet Telescope Network members. |
| pds_speclib.epn_core | Table Info | N/A | This service provides a VO version of the PDS spectral library, distributed by the PDS Geosciences node: http://pds-geosciences.wustl.edu/mro/mro-m-crism-4-speclib-v1/mrocr_90xx/ Reference: Murchie et al (2007) Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) on Mars Reconnaissance Orbiter (MRO). JGR Planets, 112:E05S03 |
| planets.epn_core | Table Info | N/A | Main characteristics of planets. Data are included in the table, therefore most relevant parameters are non-standard in EPN-TAP. Data are retrieved from Archinal et al 2018 (IAU report 2015, 2018CeMDA.130...22A) [radii] and Cox et al 2000 (Allen's astrophysical quantities, 2000asqu.book.....C) [masses, heliocentric distances, and rotation periods]. |
| planets_tuto.epn_core | Table Info | N/A | Main characteristics of planets. Data are included in the table, therefore most relevant parameters are non-standard in EPN-TAP. Data are retrieved from Archinal et al 2009 (IAU report, 2011CeMDA.109..101A) [radii] and Cox et al 2000 (Allen's astrophysical quantities, 2000asqu.book.....C) [masses, heliocentric distances, and rotation periods]. |
| posse.main | Table Info | N/A | all the image have been resampled and reprojected TAN |
| profils.epn_core | Table Info | temperature pressure and element abundancy in planetary atmosphere. | tbd |
| radiojove_hnrao_fsx8sraw.epn_core | Table Info | N/A | Radio JOVE Station HNRAO FSX8S Raw data from radio astronomy observations |
| siamama.main | Table Info | N/A | This the third step in VO-Comlpiant publication of schmidt surveys of the southern sky digitized with MAMA microdensitometer at the Observatoire de Paris Image Analysis Centre (CAI). The pixel size is 10 micrometers (0,7 arc-sec) The POSSE palomar digitized Atlas all the image have been resampled and reprojected TAN |
| spase_vespa.epn_core | Table Info | SPASE Registry catalogue mapped to EPNcore | The services provides access to the <a href="https://spase-group.org">SPASE</a> (Space Physics Archive Search and Extract) registry, as an EPNcore catalogue. |
| spectro_asteroids.epn_core | Table Info | N/A | This service provides a compilation of spectra of asteroids in the visible and NIR range. It is composed of various libraries distributed as VizieR catalogues. Reformatted VOtable or fits versions are provided with thumbnails. Ephemeris data are retrieved from Miriade (IMCCE) for the reference date when possible. |
| spectro_planets.epn_core | Table Info | N/A | This service provides a compilation of global spectra of planets and satellites in the visible and NIR range, for quick reference purpose. It is made from various libraries, including the Tohoku-Hiroshima-Nagoya Planet Spectra Library (Lundock et al 2009) and spectra from a USGS web site (R. Clark). Reformatted VOtable versions are provided together with links to the original data. |
| Tablename | Tableinfo | Table desc. | Res desc. |
| spectro_star.epn_core | Table Info | N/A | description |
| stereo_waves.epn_core | Table Info | N/A | STEREO/Waves database at LESIA. This collection contains L2 and L3 data products. This collection is maintained by the MASER team. |
| tap_schema.columns | Table Info | Columns in tables available for ADQL querying. | Unnamed data center's Table Access Protocol (TAP) service with table metadata. |
| tap_schema.groups | Table Info | Columns that are part of groups within tables available for ADQL querying. | Unnamed data center's Table Access Protocol (TAP) service with table metadata. |
| tap_schema.key_columns | Table Info | Columns participating in foreign key relationships between tables available for ADQL querying. | Unnamed data center's Table Access Protocol (TAP) service with table metadata. |
| tap_schema.keys | Table Info | Foreign key relationships between tables available for ADQL querying. | Unnamed data center's Table Access Protocol (TAP) service with table metadata. |
| tap_schema.schemas | Table Info | Schemas containing tables available for ADQL querying. | Unnamed data center's Table Access Protocol (TAP) service with table metadata. |
| tap_schema.tables | Table Info | Tables available for ADQL querying. | Unnamed data center's Table Access Protocol (TAP) service with table metadata. |
| test_datalink1.epn_core | Table Info | N/A | Demonstration service of EPN-TAP v1: main characteristics of planets. Data are included in the table, therefore most relevant parameters are non-standard in EPN-TAP. Data are retrieved from Archinal et al 2009 (IAU report, 2011CeMDA.109..101A) [radii] and Cox et al 2000 (Allen's astrophysical quantities, 2000asqu.book.....C) [masses, heliocentric distances, and rotation periods]. |
| test_datalink2.epn_core | Table Info | N/A | Demonstration service of EPN-TAP v1: main characteristics of planets. Data are included in the table, therefore most relevant parameters are non-standard in EPN-TAP. Data are retrieved from Archinal et al 2009 (IAU report, 2011CeMDA.109..101A) [radii] and Cox et al 2000 (Allen's astrophysical quantities, 2000asqu.book.....C) [masses, heliocentric distances, and rotation periods]. |
| test_datalink3.epn_core | Table Info | N/A | Demonstration service of EPN-TAP v1: main characteristics of planets. Data are included in the table, therefore most relevant parameters are non-standard in EPN-TAP. Data are retrieved from Archinal et al 2009 (IAU report, 2011CeMDA.109..101A) [radii] and Cox et al 2000 (Allen's astrophysical quantities, 2000asqu.book.....C) [masses, heliocentric distances, and rotation periods]. |
| test_hst_planeto.epn_core | Table Info | N/A | HST observations of planets, dwarf planets, and satellites, extracted from the CADC database catalogue (with daily updates). Data are linked to the CADC repository, with file names common to all HST archives. Both calibrated and derived products are included. The main target is identified. Physical ephemeris and thumbnails are provided when available. Files and previews are not accessible during the proprietary period. |
| tfcat.epn_core | Table Info | MASER/TFCat products | TFCat Database for MASER |
| tfcat.fogg_akr_wind | Table Info | TFCat table for Fogg et al. 2022 and 2023: Bursts of Auroral Kilometric Radiation individually selected from Wind/WAVES data | TFCat Database for MASER |
| tfcat.leblanc_nda_jupiter_emi | Table Info | TFCat table for Leblanc et al. A&A (1981-1993) Jupiter Radio Emissions Catalogues | TFCat Database for MASER |
| tfcat.leblanc_nda_jupiter_obs | Table Info | TFCat table for Leblanc et al. A&A (1981-1993) Jupiter Radio Observations Catalogues | TFCat Database for MASER |
| tfcat.louis_juno_waves | Table Info | TFCat table for Louis et al. JGR (2021) Jupiter Radio Emission Catalogue in Juno/Waves observations | TFCat Database for MASER |
| tfcat.marques_nda_jupiter | Table Info | TFCat table for Marques et al. A&A (2017) Jupiter Radio Emsision Catalogue | TFCat Database for MASER |
| tfcat.taubenschuss_frp_saturn | Table Info | TFCat table for Taubenschuss et al. Icarus (2021) Saturn Faraday Rotation Patches | TFCat Database for MASER |
| tfcat.wu_anomalous_nsmr | Table Info | TFCat table for Wu et al. 2022: Saturn Anomalous Myriametric Radiation, A New Type of Saturn Radio Emission Revealed by Cassini. Supplementary material: Catalogue of events | TFCat Database for MASER |
| tfcat.wu_nkom_saturn | Table Info | TFCat table for Wu et al. 2021: Statistical Study of Spatial Distribution and Polarization for Saturn Narrowband Emissions. Supplementary material: Event catalogue | TFCat Database for MASER |
| tfcat.wu_skr_harmonic | Table Info | TFCat table for Wu et al. 2022a: Catalogue of First Harmonic Saturn Kilometric Radiation Observations during Cassini’s Grand Finale | TFCat Database for MASER |
| titan_profiles.epn_core | Table Info | EPNcore table for temperature, pressure and element abundance profiles in Titan's atmosphere. | This database contains vertical profiles of temperature and composition in Titan's atmosphere at several altitudes below 750 km. These profiles were retrieved from the infrared spectra acquired by the Composite Infrared Spectrometer (CIRS) aboard the Cassini spacecraft. The retrieval method and the description of the used dataset are detailed by Vinatier et al. (2010), and completed in Mathé et al. (2020), and Vinatier et al. (2020). References ---------- - Vinatier et al. (**2010**) Analysis of Cassini/CIRS limb spectra of Titan acquired during the nominal mission: I. Hydrocarbons, nitriles and CO2 vertical mixing ratio profiles. *Icarus*, 206(2), 559-570. `doi:10.1016/j.icarus.2009.08.013 <https://doi.org/10.1016/j.icarus.2009.08.013>`_ - Mathé et al. (**2020**) Seasonal changes in the middle atmosphere of Titan from Cassini/CIRS observations: Temperature and trace species abundance profiles from 2004 to 2017. *Icarus*, 344, 113547. `doi:10.1016/j.icarus.2019.113547 <https://doi.org/10.1016/j.icarus.2019.113547>`_ - Vinatier et al. (**2020**), Temperature and chemical species distributions in the middle atmosphere observed during Titan's late northern spring to early summer. A&A 641, A116; `doi:10.1051/0004-6361/202038411 <https://doi.org/10.1051/0004-6361/202038411>`_ |
| tnosarecool.epn_core | Table Info | N/A | This service lists TNO thermal properties as derived mostly from Spitzer and Herschel observations. |
| ufe.main | Table Info | N/A | TBD |
| Tablename | Tableinfo | Table desc. | Res desc. |
| usgs_wms.epn_core | Table Info | Catalogue of USGS Astrogeology WMS Map Layers | EPN-TAP access to a selection of Astrogeology WMS Map Layers listed at https://astrowebmaps.wr.usgs.gov/webmapatlas/Layers/maps.html. These layers are exposed via https://planetarymaps.usgs.gov/ The database lists various global mosaics for most planetary bodies in the Solar System. The field external_link contains a link to a WMS web viewer for that map. The field access_url contains a link to the GetCapabilities request for the server, which serves as an endpoint for interfacing with QGIS. Hare, T. M., et al. 2014 "Online Planetary Data and Services at USGS Astrogeology", Lunar and Planetary Science Conference 45. |
| vims_satellites.epn_core | Table Info | N/A | The Visual and Infrared Mapping Spectrometer (VIMS) instrument onboard the Cassini spacecraft observed the system of Saturn, acquiring spectral cubes in the range 0.4-5.2 microns. This service focuses on Saturn satellites, and provides access to calibrated and ancillary data, computed as described here: https://vims.univ-nantes.fr/info/isis-calibration. It also provides direct links to a larger web site with previews. |
| vispecstar.epn_core | Table Info | N/A | description |
| VOccDB.epn_core | Table Info | N/A | The VOccDB database provides prediction and parameters of stellar occultations by the main planetary satellites. Observations of a stellar occultations help to better determine the size and the shape of the occulting body, as well as its astrometric position at the milli-arcsecond level precision. Only the main moons of giant planets Jupiter, Saturn, Uranus and Neptune are considered in the event prediction database. Predictions are provided over period 2023-2032, up to visual magnitude 12 for the biggest satellites, and magnitude 14 for other satellites. For each stellar occultation event prediction, the database provides circumstances and observational data, date and timing of the occultation, star position and magnitude, excepted duration, etc. |
| voyager_pra.epn_core | Table Info | N/A | Voyager PRA (Planetary Radio Astronomy) Datasets catalog. The dataset are originally published by several data centers: NASA/PDS, NASA/NSSDC, NASA/GSFC, Univ. Iowa and CNES/SERAD. |
| vvex_db.epn_core | Table Info | IR spectroscopy of Venus | VIRTIS/Venus Express demonstrator service: imaging spectroscopy of Venus in the visible and the near infrared. Assessment version from PI team database. |
| vvex.epn_core | Table Info | IR spectroscopy of Venus | VIRTIS/Venus Express demonstrator service: imaging spectroscopy of Venus in the visible and the near infrared. ** Assessment version from PI team database - some values currently missing ** This lists all calibrated files for the total mission and the three channels M-vis, M-IR and H. Files are described according to the PI team database, with links to the PSA: https://archives.esac.esa.int/psa/ftp/VENUS-EXPRESS/VIRTIS/VEX-V-VIRTIS-2-3-V3.0/. See Piccioni et al, 2007, VIRTIS: The Visible and Infrared Thermal Imaging Spectrometer, ESA SP 1295. |
| vvex_test.epn_core | Table Info | IR spectroscopy of Venus | VIRTIS/Venus Express demonstrator service: imaging spectroscopy of Venus in the visible and the near infrared. ** Assessment version from PI team database - some values currently missing ** This lists all calibrated files for the total mission and the three channels M-vis, M-IR and H. Files are described according to the PI team database, with links to the PSA: https://archives.esac.esa.int/psa/ftp/VENUS-EXPRESS/VIRTIS/VEX-V-VIRTIS-2-3-V3.0/. See Piccioni et al, 2007, VIRTIS: The Visible and Infrared Thermal Imaging Spectrometer, ESA SP 1295. |
| wind_waves.epn_core | Table Info | VESPA/Epncore table for the Wind/Waves LESIA Database | Wind/Waves LESIA Database |